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101.
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Yong Yu Xiao-Fen Zhao Hao Luo Yin-Dun Mao Zheng-Hong Tang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2320-2327
Geosynchronous Earth Orbit (GEO) satellites are widely used because of their unique characteristics of high-orbit and remaining permanently in the same area of the sky. Precise monitoring of GEO satellites can provide a key reference for the judgment of satellite operation status, the capture and identification of targets, and the analysis of collision warning. The observation using ground-based optical telescopes plays an important role in the field of monitoring GEO targets. Different from distant celestial bodies, there is a relative movement between the GEO target and the background reference stars, which makes the conventional observation method limited for long focal length telescopes. CCD drift-scan photoelectric technique is applied on monitoring GEO targets. In the case of parking the telescope, the good round images of the background reference stars and the GEO target at the same sky region can be obtained through the alternating observation of CCD drift-scan mode and CCD stare mode, so as to improve the precision of celestial positioning for the GEO target. Observation experiments of GEO targets were carried out with 1.56-meter telescope of Shanghai Astronomical Observatory. The results show that the application of CCD drift-scan photoelectric technique makes the precision of observing the GEO target reach the level of 0.2″, which gives full play to the advantage of the long focal length of the telescope. The effect of orbit improvement based on multi-pass of observations is obvious and the prediction precision of extrapolating to 72-h is in the order of several arc seconds in azimuth and elevation. 相似文献
104.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(10):2315-2323
This paper presents the mechanical design of a new robotic telescope that was designed and built to acquire lunar spectral measurements from the science pod of NASA's ER-2 aircraft while flying at an altitude of 70,000 feet (21.34 km). The robotic telescope used a double gimbal design that allowed for target tracking in azimuth and elevation. In addition to the challenging and restrictive geometry of the science pod, each component needed to be carefully selected to ensure that they could withstand the operating conditions at high altitude such as harsh temperatures extending as low as −54 °C and atmospheric pressure less than 1.05 psi (7.23 kPa). Due to the cold temperatures, low atmospheric pressure and the likely exposure to moisture, high strength industrial linear actuators were used to create an adjustable linkage system that controlled the pointing and tracking of the telescope. Although unconventional, this allowed for a robust design that outperformed the team's expectations by tracking the Moon for 40 min with an average tracking error under 0.05°. The results presented within this paper were acquired during a first set of engineering test flights, with further scientific missions to follow. 相似文献
105.
Pankaj K. Soni Bharati Kakad Amar Kakad 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(2):749-761
This article aims to understand the motion of the charged particles trapped in the Earth’s inner magnetosphere. The emphasis is on identifying the numerical scheme, which is appropriate to characterize the trajectories of the charged particles of different energies that enter the Earth’s magnetosphere and get trap along the magnetic field lines. These particles perform three different periodic motions, namely: gyration, bounce, and azimuthal drift. However, often, the gyration of the particle is ignored, and only the guiding center of the particle is traced to reduce the computational time. It is because the simulation of all three motions (gyro, bounce, and drift) together needed a robust numerical scheme, which has less numerical dissipation. We have developed a three-dimensional test particle simulation model in which the relativistic equation of motion is solved numerically using the fourth and sixth-order Runge-Kutta methods. The stability of the simulation model is verified by checking the conservation of total kinetic energy and adiabatic invariants linked with each type of motion. We found that the sixth-order Runge-Kutta method is suitable to trace the complete trajectories of both proton and electron of a wide energy range, 5 keV to 250 MeV for L = 2 – 6. We have estimated the bounce and drift periods from the simulations, and they are found to be in good agreement with the theory. The study implies that a simulation model with sixth-order Runge-Kutta method can be applied to the time-vary, non-analytical form of magnetic configuration in future studies to understand the dynamics of charged particles trapped in Earth’s magnetosphere. 相似文献
106.
介绍了航天器的热控制模式、对在微重力下的单相流与两相流的换热系统、微重力下与重力场下的两相流沸腾换热进行了比较。最后论述了在微重力条件下进行两相流沸腾换热地面等效试验研究的必要性。 相似文献
107.
The energy state of a planet depends fundamentally on its radiation budget. Measurements made from space over past decades
have led to significant revisions of ground-based estimates, both of the reflected fraction (the Bond albedo) of solar radiative
flux and of the emitted thermal infrared radiation flux, for the Earth as well as for the other planets. After a brief survey
of methods and difficulties in accurately determining planetary radiation budgets, we note contradictions in existing tabulations
of global parameters, in particular Bond albedo. For the Earth, such contradictions are unjustified, considering that global
and annual means as well as the seasonal cycle of Earth Radiation Budget components have now been determined with high accuracy.
The Earth's Bond albedo is close to 0.3. Net storage of energy in the Earth-ocean system is close to zero, with a well-established
annual cycle of amplitude close to ±12 Wm−2. Some contradictions remain for the other terrestrial planets. For the giant planets, modern reduced values of the Bond albedo
imply reduced but still significant internal energy generation. 相似文献
108.
109.
在中轨卫星移动通信系统中 ,确定小区驻留时间分布对于合理地规划切换策略具有十分重要的意义。文中指出了地球固定覆盖与卫星固定覆盖两种方式下小区驻留时间分布不同的原因。提出一种仿真计算卫星固定覆盖方式下小区驻留时间分布的方法 ,得出了数值结果 ,并与地球固定覆盖方式下的小区驻留时间分布作了比较 相似文献
110.
本文讨论了地球扁率引起红外地平仪的姿态量测误差的数学模型,导出解析形式姿态误差计算公式,可在任意轨道根数和扫描轴安装角情况下用于误差补偿。算例表明,利用本文导出的解析公式与利用数值方法的计算结果完全一致。 相似文献